The Allen Telescope Array Twenty-centimeter Survey—A - CIRA
The Allen Telescope Array Twenty-centimeter Survey—A - CIRA
The Allen Telescope Array Twenty-centimeter Survey—A - CIRA
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– 26 –<br />
Fig. 12.— Left: Positional offsets in RA and Dec for sources detected by both NVSS and<br />
ATATS. Right: Histogram of offsets ( ∆RA 2 +∆Dec 2 ) for sources detected by both NVSS<br />
and ATATS. <strong>The</strong> majority of the matches fall within a radius corresponding to the ATA<br />
synthesized beam (∼ 75 ′′ ) – those at larger radii are mostly spurious matches of an NVSS<br />
source with an unassociated nearby ATA source, where the true match was not detected by<br />
the ATA.